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THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY
- Source :
- Abazajian, K N, Adelman-McCarthy, J K, Agueros, M A, Allam, S S, Allende Prieto, C, An, D, Anderson, K S J, Anderson, S F, Annis, J, Bahcall, N A, Bailer-Jones, C A L, Barentine, J C, Bassett, B A, Becker, A C, Beers, T C, Bell, E F, Belokurov, V, Berlind, A A, Berman, E F, Bernardi, M, Bickerton, S J, Bizyaev, D, Blakeslee, J P, Blanton, M R, Bochanski, J J, Boroski, W N, Brewington, H J, Brinchmann, J, Brinkmann, J V, Brunner, R J, Budavari, T, Carey, L N, Carliles, S, Carr, M A, Castander, F J, Cinabro, D, Connolly, A J, Csabai, I, Cunha, C E, Czarapata, P C, Davenport, J R A, de Haas, E, Dilday, B, Doi, M, Eisenstein, D J, Evans, M L, Evans, N W, Fan, X, Friedman, S D, Frieman, J A, Fukugita, M, Gansicke, B T, Gates, E, Gillespie, B A, Gilmore, G, Gonzalez, B, Gonzalez, C F, Grebel, E K, Gunn, J E, Gyory, Z, Hall, P B, Harding, P, Harris, F H, Harvanek, M, Hawley, S L, Hayes, J J E, Heckman, T M, Hendry, J S, Hennessy, G S, Hindsley, R B, Hoblitt, J, Hogan, C J, Hogg, D W, Holtzman, J A, Hyde, J B, Ichikawa, S, Ichikawa, T, Im, M, Ivezic, Z, Jester, S, Jiang, L, Johnson, J A, Jorgensen, A M, Juric, M, Kent, S M, Kessler, R, Kleinman, S J, Knapp, G R, Konishi, K, Kron, R G, Krzesinski, J, Kuropatkin, N, Lampeitl, H, Lebedeva, S, Lee, M G, Lee, Y S, Leger, R F, Lepine, S, Li, N, Lima, M, Lin, H, Long, D C, Loomis, C P, Loveday, J, Lupton, R H, Magnier, E, Malanushenko, O, Malanushenko, V, Mandelbaum, R, Margon, B, Marriner, J P, Martinez-Delgado, D, Matsubara, T, McGehee, P M, McKay, T A, Meiksin, A, Morrison, H L, Mullally, F, Munn, J A, Murphy, T, Nash, T, Nebot, A, Neilsen, E H J, Newberg, H J, Newman, P R, Nichol, R C, Nicinski, T, Nieto-Santisteban, M, Nitta, A, Okamura, S, Oravetz, D J, Ostriker, J P, Owen, R, Padmanabhan, N, Pan, K, Park, C, Pauls, G, Peoples, J J, Percival, W J, Pier, J R, Pope, A C, Pourbaix, D, Price, P A, Purger, N, Quinn, T, Raddick, M J, Fiorentin, P R, Richards, G T, Richmond, M W, Riess, A G, Rix, H-W, Rockosi, C M, Sako, M, Schlegel, D J, Schneider, D P, Scholz, R-D, Schreiber, M R, Schwope, A D, Seljak, U, Sesar, B, Sheldon, E S, Shimasaku, K, Sibley, V C, Simmons, A E, Sivarani, T, Smith, J A, Smith, M C, Smolcic, V, Snedden, S A, Stebbins, A, Steinmetz, M, Stoughton, C, Strauss, M A, Subbarao, M, Suto, Y, Szalay, A S, Szapudi, I, Szkody, P, Tanaka, M, Tegmark, M, Teodoro, L F A, Thakar, A R, Tremonti, C A, Tucker, D L, Uomoto, A, Vanden Berk, D E, Vandenberg, J, Vidrih, S, Vogeley, M S, Voges, W, Vogt, N P, Wadadekar, Y, Watters, S, Weinberg, D H, West, A A, White, S D M, Wilhite, B C, Wonders, A C, Yanny, B, Yocum, D R, York, D G, Zehavi, I, Zibetti, S & Zucker, D B 2009, ' The seventh data release of the Sloan Digital Sky Survey ', The Astrophysical Journal Supplement Series, vol. 182, no. 2, pp. 543-558 . https://doi.org/10.1088/0067-0049/182/2/543
- Publication Year :
- 2009
- Publisher :
- American Astronomical Society, 2009.
-
Abstract
- This paper describes the Seventh Data Release of the Sloan Digital Sky Survey (SDSS), marking the completion of the original goals of the SDSS and the end of the phase known as SDSS-II. It includes 11663 deg^2 of imaging data, with most of the roughly 2000 deg^2 increment over the previous data release lying in regions of low Galactic latitude. The catalog contains five-band photometry for 357 million distinct objects. The survey also includes repeat photometry over 250 deg^2 along the Celestial Equator in the Southern Galactic Cap. A coaddition of these data goes roughly two magnitudes fainter than the main survey. The spectroscopy is now complete over a contiguous area of 7500 deg^2 in the Northern Galactic Cap, closing the gap that was present in previous data releases. There are over 1.6 million spectra in total, including 930,000 galaxies, 120,000 quasars, and 460,000 stars. The data release includes improved stellar photometry at low Galactic latitude. The astrometry has all been recalibrated with the second version of the USNO CCD Astrograph Catalog (UCAC-2), reducing the rms statistical errors at the bright end to 45 milli-arcseconds per coordinate. A systematic error in bright galaxy photometr is less severe than previously reported for the majority of galaxies. Finally, we describe a series of improvements to the spectroscopic reductions, including better flat-fielding and improved wavelength calibration at the blue end, better processing of objects with extremely strong narrow emission lines, and an improved determination of stellar metallicities. (Abridged)<br />Comment: 20 pages, 10 embedded figures. Accepted to ApJS after minor corrections
- Subjects :
- Cosmology and Gravitation
Astronomy
media_common.quotation_subject
FOS: Physical sciences
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics
atlases
catalogs
surveys
law.invention
Photometry (optics)
law
Astrophysics::Solar and Stellar Astrophysics
Astrophysics::Galaxy Astrophysics
media_common
Physics
Imaging systems in astronomy
Stars--Observations
Celestial equator
Astrophysics (astro-ph)
Astrophysics::Instrumentation and Methods for Astrophysics
Astronomy and Astrophysics
Quasar
Astrometry
Astrograph
Galaxy
Stars
Space and Planetary Science
Sky
Subjects
Details
- ISSN :
- 15384365 and 00670049
- Volume :
- 182
- Database :
- OpenAIRE
- Journal :
- The Astrophysical Journal Supplement Series
- Accession number :
- edsair.doi.dedup.....6ec03b70e4fb97702a8c4902c94288ec